All Posters

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Session 1 - Solar magnetic variability and irradiance over the solar cycle

Conveners: Marc DeRosa (LMSAL), Jesper Schou (MPS)

The solar dynamo: Inferences from observationsCameron, R
Delayed Babcock-Leighton dynamos with high diffusion.Fournier, Y
Study of Ionosphere Variability over equatorial latitude during extreme low solar activity periodPurohit, D
The Sunspot Number recalibrationLefevre, L
Measurements of Solar Oblateness during the SDO MissionBush, R
Soothing Massage of HMI Magnetic Field DataHoeksema, T
On the acoustic mode frequency dependence with solar cycleRabello soares, M
Tracking of predominant periodicities evolution for PROBA2/LYRA and other long-term solar time seriesWauters, L
The photospheric structure of coronal holes: magnetic elementsHofmeister, S

Session 2 - Precursors and signatures of eruptive events

Conveners: Barbara Thompson (GSFC), James Mason (GSFC)

Spatiotemporal Heliomarker Discovery from Spatiotemporal Frequent PatternsAydin, B
A study on the relationship between hard X-ray emission and magnetic field changes during solar flaresCaicedo, W
Detection of Three-minute Oscillations in Full-disk Lyman-alpha Emission during a Solar FlareMilligan, R
Multi-wavelength observations of 4 homologous global coronal wavesLong, D
AWARE: An algorithm for the automated characterization of EUV waves in the solar atmosphereIreland, J
Understanding the Role of Mass-Unloading in a Filament EruptionLong, D
Oscillations along Flare Loops in Multiple Wavelengths and their Correlations to Photospheric WavesHess webber, S
Dynamic Mapping of Solar EruptionsThompson, B
On the Magnetic Topology and Extreme Ultraviolet in Solar Flares with Late PhaseChen, J
A Truly Global Extreme Ultraviolet Wave from the SOL2017-09-10 X8.2+ Solar Flare-Coronal Mass EjectionLiu, W
Estimation of Halo CME’s radial speeds using coronal shock waves based on SDO/AIA observationsJeong, H
Effect of transport coefficients on excitation of flare-induced standing slow-mode waves in coronal loopsWang, T

Session 3 - Subsurface motions and flows

Conveners: Dean Pesnell (GSFC), Rebecca Centeno (HAO/NCAR)

On the depth dependence of solar equatorial Rossby wavesProxauf, B
First comprehensive calculation of the whole solar convection zoneHotta, H
Subsurface Flows During Cycle 23 and 24Komm, R
The HMI Ring-Diagram Pipeline: Recent Developments and Future ProspectsBogart, R
The Minimum Energy Principle Applied to Parker's Coronal Braiding and Nanoflaring ScenarioAschwanden, M
Interactions of waves with solar convectionSchou, J
Rossby waves in the solar convection zone measured by deep-focus time-distance helioseismologyDuvall, T
Towards improved multi-ridge fitting method for ring-diagram analysis Nagashima, K
Impact of observational duty cycle on the measurement of local helioseismic mode parametersTripathy, S
A New Approach for Calculating Three-Dimensional Flow Sensitivity Kernels Using Global-Scale Wavefield SimulationsZhao, J
Statistical Analysis of Acoustic Wave Power and Flows around Solar Active RegionsRabello soares, M
Near-Surface Flow Anomalies in Solar Cycle 24 As Determined By Ring-Diagram AnalysisBaldner, C
A fragile detection of solar g-modesSchunker, H

Session 4 - Data-driven modeling of solar atmosphere and solar explosive events

Conveners: Meng Jin (LMSAL), Véronique Delouille (ROB)

Soft X-ray (0.1 – 2.5 nm) Spectral Emission Lines Associated with AR 12713 Observed with Rocket EVE/SAM Instrument on June 18, 2018Didkovsky, L
Observations and Modeling of a High-Latitude, Extended Filament Channel EruptionLynch, B
Global Magnetohydrodynamics Simulation of EUV Waves and Shocks from the X8.2 Eruptive Flare on 2017 September 10Jin, M
Fast velocities of flare ribbon kernels and ribbon elongation in a quiescent filament eruption of 2012 August 31 observed by SDO/AIALorincik, J
Eruptions from quiet Sun coronal bright points: Observations & ModelingMadjarska-theissen, M
On the extrapolation of magneto-hydro-static equilibria on the sun: model and testsZhu, X
What can we learn from impulsively generated waves observed by SDO/AIA?Ofman, L
Research on Solar Drivers of Space-weather: Sun-Earth connection of magnetic flux ropesVemareddy, P

Session 5 - Frontier: Solar Poles Exploration and new prospects

Conveners: Rebecca Centeno (HAO/NCAR), Barbara Thompson (GSFC)

Exploring The Solar Poles From L1 PerspectiveWest, M
New HMI Data Series: temporally consistent disambiguation for HARP vector magnetic field timeseries dataBarnes, G
NuSTAR’s observations of tiny flares and big eruptions Hannah, I
The butterfly diagram and tilt angles obtained from the Horrebow sunspot observationsValliappan, S
The Role of the Solar Soft X-ray Irradiance on Thermospheric Chemistry and StructureSamaddar, S
New and Improved Mode Fitting ResultsKorzennik, S
Variation in Sun's Seismic Radius and its implication on the TSI variabilityTripathy, S

Session 6 - Magnetic structure of the corona and its transition to the heliosphere

Conveners: David Berghmans (ROB), Marc DeRosa (LMSAL)

Exceptional Extended Field of View Observations by SWAP on 1 and 3 April 2017O'hara, J
Solar Coronal Jets Extending beyond the AIA Field of View Observed during the 2017 August 21Hanaoka, Y
Long-term evolution of the solar corona using SWAP dataMierla, M
Reflection of Acoustic Modes on SunspotsWaidele, M
Power spectrum power-law indices as a diagnostic of coronal heatingIreland, J
On the Vertical Magnetic Field at the Umbral Boundary of a long-lived SunspotSchmassmann, M
Multi-wavelength Observations of Flare-Induced Acoustic Waves Around Active Regions with SDO AIAPesnell, D
The spectral content of SDO/AIA 1600 and 1700 A filters from flare and plage observationsMilligan, R

Session 7 - Machine Learning and Forecasting

Conveners: Véronique Delouille (ROB), Meng Jin (LMSAL)

Supervised Neural Networks for Helioseismic Ring-diagram InversionsHanson, C
Extracting Solar Physics from 151 Million EUV ImagesKirk, M
Irradiance Coronal Dimming and its Connection to CME KineticsMason, J
Coronal holes detection using supervised classificationDelouille, V
Driving Scientific Discovery with Machine Learning and AI at the NASA GSFC Center for HelioAnalyticsThompson, B
SHARPs and SMARPs: 22 years of solar active region dataBobra, M
Estimating solar far-side magnetic flux from STEREO EUV observations by deep learningChen, R
Photospheric Magnetic Field Properties of Flaring vs. Flare-quiet active regions, V: Results from HMILeka, K
A deep learning approach to forecast tomorrow's solar wind parameters.Shneider, C
AI-generated EUV images from SDO/HMI magnetograms by deep learningPark, E
Combining sparsity DEM inversions with event tracking for AIA dataBethge, C

Session 8 - Solar/stellar magnetic activity and its influence on planetary bodies

Conveners: James Mason (GSFC), Marc DeRosa (LMSAL)

Latitudinal variability of Total electron content over low, mid and high latitudes during solar maximum and its comparison with IRI-2012 and IRI-2016 modelAtulkar, R
Stellar activity effects on high energy exoplanet transitsLlama, J
Astrospheric Space Weather as a Factor of (Exo)Planetary HabitabilityAirapetian, V

Session 9 - Tool market

Conveners: Barbara Thompson (GSFC), Dean Pesnell (GSFC)

New developments and applications of Helioviewer Project servicesIreland, J
sTools - a software package for data reduction of GREGOR instruments and general data analysisDiercke, A
The SDO AIA and HMI archive at MEDOCBuchlin, E
SDO-EVE Data Download and Processing Using SunPy©Templeman, B
NASA Rocket 36.336 Extreme Ultraviolet SpectrumWoodraska, D
The NASA Space Science Education Consortium (NSSEC)Young, A
Low Latency Space Weather Products from SDO-EVEJones, A